γ-Ray Observations from the OSO-3 satellite

Details γ-Ray Observations from the OSO-3 satellite γ-Ray Observations from the OSO-3 satellite

Mar 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..27..147b&link_type=abstract

Astrophysics and Space Science, Volume 27, Issue 1, pp.147-155

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

The result on λ-rays obtained from the analysis of 5800 orbits of data from the University of Rochester telescope on board the OSO-3 satellite are presented. For γ-rays of energy greater than 100 MeV, an upper limit of 2.3×10-4 cm-2 s-1 std has been placed on the diffuse (assumed isotropic) flux. An upper limit to the flux from the Sun is set at 3.2×10-5 and 2.4×10-5 cm-2 s-1 for energies greater than 50 MeV and 100 MeV, respectively. All flux values are calculated assuming a π0-decay source of γ-rays.

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